-
4
-
-
12044251032
-
-
E. Dagotto, Rev. Mod. Phys. 66, 763 (1994), and references cited therein.
-
(1994)
Rev. Mod. Phys.
, vol.66
, pp. 763
-
-
Dagotto, E.1
-
10
-
-
11644278718
-
-
M. Langer, J. Schmalian, S. Grabowski and K.H. Bennemann, Phys. Rev. Lett. 75, 4508 (1995).
-
(1995)
Phys. Rev. Lett.
, vol.75
, pp. 4508
-
-
Langer, M.1
Schmalian, J.2
Grabowski, S.3
Bennemann, K.4
-
11
-
-
4243170741
-
-
A. Fujimori, I. Hase, H. Namatame, Y. Fujishima, Y. Tokura, H. Eisaki, S. Uchida, K. Takegahara and F.M.F. de Groot, Phys. Rev. Lett. 69, 1796 (1992).
-
(1992)
Phys. Rev. Lett.
, vol.69
, pp. 1796
-
-
Fujimori, A.1
Hase, I.2
Namatame, H.3
Fujishima, Y.4
Tokura, Y.5
Eisaki, H.6
Uchida, S.7
Takegahara, K.8
de Groot, F.9
-
12
-
-
11944254048
-
-
I.H. Inoue, I. Hase, Y. Aiura, A. Fujimori, Y. Haruyama, T. Maruyama and Y. Nishihara, Phys. Rev. Lett. 74, 2539 (1995).
-
(1995)
Phys. Rev. Lett.
, vol.74
, pp. 2539
-
-
Inoue, I.1
Hase, I.2
Aiura, Y.3
Fujimori, A.4
Haruyama, Y.5
Maruyama, T.6
Nishihara, Y.7
-
13
-
-
0000659088
-
-
K. Morikawa, T. Mizokawa, K. Kobayashi, A. Fujimori, H. Eisaki, S. Uchida, F. Iga and Y. Nishihara, Phys. Rev. B 52, 13t711 (1995).
-
(1995)
Phys. Rev. B
, vol.52
, pp. 13711
-
-
Morikawa, K.1
Mizokawa, T.2
Kobayashi, K.3
Fujimori, A.4
Eisaki, H.5
Uchida, S.6
Iga, F.7
Nishihara, Y.8
-
18
-
-
0000386712
-
-
A. Fujimori, I. Hase, M. Nakamura, H. Namatame, Y. Fujishima, Y. Tokura, M. Abbate, F.M.F. de Groot, J.C. Fuggle, O. Strebel, M. Doce and G. Kaindl, Phys. Rev. B 46, 9841 (1992).
-
(1992)
Phys. Rev. B
, vol.46
, pp. 9841
-
-
Fujimori, A.1
Hase, I.2
Nakamura, M.3
Namatame, H.4
Fujishima, Y.5
Tokura, Y.6
Abbate, M.7
de Groot, F.8
Fuggle, J.9
Strebel, O.10
Doce, M.11
Kaindl, G.12
-
19
-
-
3242875501
-
-
Y. Tokura, Y. Taguchi, Y. Okada, Y. Fujishima, T. Arima, K. Kumagai and Y. Iye, Phys. Rev. Lett. 70, 2126 (1993).
-
(1993)
Phys. Rev. Lett.
, vol.70
, pp. 2126
-
-
Tokura, Y.1
Taguchi, Y.2
Okada, Y.3
Fujishima, Y.4
Arima, T.5
Kumagai, K.6
Iye, Y.7
-
22
-
-
0030528685
-
-
For a review, see A. Georges, G. Kotliar, W. Krauth and M. Rozenberg, Rev. Mod. Phys. 68, 13 (1996).
-
(1996)
Rev. Mod. Phys.
, vol.68
, pp. 13
-
-
Georges, A.1
Kotliar, G.2
Krauth, W.3
Rozenberg, M.4
-
25
-
-
25044438103
-
-
S.R. White, D.J. Scalapino, R.L. Sugar, E.Y. Loh, J.E. Gubernatis and R.T. Scalettar, Phys. Rev. B 40, 506 (1989).
-
(1989)
Phys. Rev.
, vol.B40
, pp. 506
-
-
White, S.1
Scalapino, D.2
Sugar, R.3
Loh, E.4
Gubernatis, J.5
Scalettar, R.6
-
28
-
-
33744704058
-
-
R.T. Scalettar, D.J. Scalapino, R.L. Sugar and D. Toussaint, Phys. Rev. B 39, 4711 (1989).
-
(1989)
Phys. Rev. B
, vol.39
, pp. 4711
-
-
Scalettar, R.1
Scalapino, D.2
Sugar, R.3
Toussaint, D.4
-
32
-
-
33749414347
-
-
A. Moreo et. al Phys. Rev. B 51, 12t045 (1995).
-
(1995)
Phys. Rev. B
, vol.51
, pp. 12045
-
-
Moreo, A.1
-
38
-
-
33749415529
-
-
D.D. Sarma et. al Phys. Rev. B 49, 14t238 (1994).
-
(1994)
Phys. Rev. B
, vol.49
, pp. 14238
-
-
Sarma, D.1
-
40
-
-
0000773196
-
-
M.J. Rozenberg, G. Kotliar, H. Kajueter, G.A. Thomas, D.H. Rapkine, J.M. Honig and P. Metcalf, Phys. Rev. Lett. 75, 105 (1995).
-
(1995)
Phys. Rev. Lett.
, vol.75
, pp. 105
-
-
Rozenberg, M.1
Kotliar, G.2
Kajueter, H.3
Thomas, G.4
Rapkine, D.5
Honig, J.6
Metcalf, P.7
-
43
-
-
0001451747
-
-
The self-consistent perturbation theory around the SDW MF solution provides a renormalization factor about q=0.29 in the limit of small U in D=3 and D=∞. Numerically it was found that q increases with U, see, e.g., Ref. 12
-
P. van Dongen, Phys. Rev. Lett. 67, 757 (1991). The self-consistent perturbation theory around the SDW MF solution provides a renormalization factor about q=0.29 in the limit of small U in D=3 and D=∞. Numerically it was found that q increases with U, see, e.g., Ref. 12.
-
(1991)
Phys. Rev. Lett.
, vol.67
, pp. 757
-
-
van Dongen, P.1
-
45
-
-
0001215723
-
-
F. Marsiglio, A.E. Ruckenstein, S. Schmitt-Rink and C.M. Varma, Phys. Rev. B 43, 10t882 (1991).
-
(1991)
Phys. Rev. B
, vol.43
, pp. 10882
-
-
Marsiglio, F.1
Ruckenstein, A.2
Schmitt-Rink, S.3
Varma, C.4
-
51
-
-
3342922278
-
-
Recently proposed theories of high (Formula presented) make extensive use of a large accumulation of weight in the DOS near the chemical potential to enhance the critical temperature [E. Dagotto, A. Nazarenko and A. Moreo, Phys. Rev. Lett. 74, 310 (1995)].
-
(1995)
Phys. Rev. Lett.
, vol.74
, pp. 310
-
-
Dagotto, E.1
Nazarenko, A.2
Moreo, A.3
-
55
-
-
0003882925
-
-
A.Y. Matsuura, Z.-X. Shen, D.S. Dessau, C.-H. Park, T. Thio, J. W. Bennett and O. Jepson, Phys. Rev. B 53, R7584 (1996).
-
(1996)
Phys. Rev. B
, vol.53
, pp. R7584
-
-
Matsuura, A.1
Dessau, D.2
Thio, T.3
Bennett, J.4
Jepson, O.5
-
56
-
-
7544235845
-
-
M.J. Rozenberg, I.H. Inoue, H. Makino, F. Iga and Y. Nashihara, Phys. Rev. Lett. 76, 4781 (1996).
-
(1996)
Phys. Rev. Lett.
, vol.76
, pp. 4781
-
-
Rozenberg, M.1
Inoue, I.2
Makino, H.3
Iga, F.4
Nashihara, Y.5
-
57
-
-
4243153248
-
-
E. Dagotto, J. Riera, A. Sandvik and A. Moreo, Phys. Rev. Lett. 76, 1731 (1996).
-
(1996)
Phys. Rev. Lett.
, vol.76
, pp. 1731
-
-
Dagotto, E.1
Riera, J.2
Sandvik, A.3
Moreo, A.4
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